THE NUMERICAL SIMULATION OF PERTURBED ACCRETION DISK AROUND THE MASSIVE BLACK HOLE

DOI10.1142/S0218271806008735zbMath1119.85004MaRDI QIDQ3430404

Orhan Dönmez

Publication date: 21 March 2007

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

zbMATH Keywords

general relativityhydrodynamicsX-raynumerical relativity black holespiral shockperturbed accretion disk

Mathematics Subject Classification ID

Galactic and stellar structure (85A15)

Cites Work

• Code development of three-dimensional general relativistic hydrodynamics with AMR (Adaptive-Mesh Refinement) and results from special and general relativistic hydrodynamics
• Numerical simulation of rotating accretion disk around the Schwarzschild black hole using GRH code
• Gravitating discs around black holes

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